GCN Guidelines for ePESSTO reporting of GRB observations

In this case we should put the observers first, then the GRB science team who analysed and wrote the GCN, then ePESSTO Builders list and the on-duty team for that subrun (the TAT on duty and the data analysis team).

MAIN TEXT:

We observed GRB YYMMDDA under the the extended Public ESO Spectroscopic Survey for Transient Objects (ePESSTO; see Smartt et al. 2015, A&A, 579, 40 http://www.pessto.org ). The observations were performed on the ESO New Technology Telescope at La Silla with the EFOSC2/SofI instrument in spectroscopic/imaging mode starting from YYYY-MM-DD at HH:MM:SS UT (i.e. XX.X hours from the burst).

Followed by a paragraph describing the results (afterglow detection/upper limit, redshift based on absorption/emission lines identification in the spectrum.